Rumuruti meteorite NWA 13685 - 276 g






Over 20 years collecting meteorites; former museum curator and experienced restorer.
| €350 | ||
|---|---|---|
| €100 | ||
| €3 | ||
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Rumuruti meteorite, a stony meteorite of type NWA 13685 from Mauritania, weighing 276 g and described as a crusted piece.
Description from the seller
Nice piece of rocky meteorite, Rumuruti-type, a piece with original crust and the fantastic chondrules.
Rumuruti chondrites are a very rare type of chondrites. Less than 0.5% of the chondrites are classified as R.
They differ from ordinary chondrites mainly in having most of the metal in the form of sulfides, in being more oxidized, and in containing little iron and nickel metal.
They have a matrix with more dust (about 50%), a higher concentration of trace elements zinc and selenium, and a higher proportion of oxygen-17 than ordinary chondrites.
They are called "R" after the Rumuruti meteorite, which fell on January 28, 1934 in the Rift Valley, Kenya.
Chondrites are the oldest materials in the solar system, with an estimated formation age of 4.550 billion years. They are meteorites that have not undergone differentiation, which is why they contain iron, in this case in small amounts since they are LL-type.
Most of them come from the asteroid belt located between the planets Mars and Jupiter.
The characteristic feature of chondrites is the presence of chondrules, small, millimeter-sized spheres composed largely of silicates.
The standard model for their initial formation is that they form during the condensation of the solar nebula from cosmic dust.
Chondrites are the earliest building blocks from which planets form.
At Expometeoritos, we handle outreach, talks, workshops, analyses, classification, and exhibitions of meteorites.
Seller's Story
Nice piece of rocky meteorite, Rumuruti-type, a piece with original crust and the fantastic chondrules.
Rumuruti chondrites are a very rare type of chondrites. Less than 0.5% of the chondrites are classified as R.
They differ from ordinary chondrites mainly in having most of the metal in the form of sulfides, in being more oxidized, and in containing little iron and nickel metal.
They have a matrix with more dust (about 50%), a higher concentration of trace elements zinc and selenium, and a higher proportion of oxygen-17 than ordinary chondrites.
They are called "R" after the Rumuruti meteorite, which fell on January 28, 1934 in the Rift Valley, Kenya.
Chondrites are the oldest materials in the solar system, with an estimated formation age of 4.550 billion years. They are meteorites that have not undergone differentiation, which is why they contain iron, in this case in small amounts since they are LL-type.
Most of them come from the asteroid belt located between the planets Mars and Jupiter.
The characteristic feature of chondrites is the presence of chondrules, small, millimeter-sized spheres composed largely of silicates.
The standard model for their initial formation is that they form during the condensation of the solar nebula from cosmic dust.
Chondrites are the earliest building blocks from which planets form.
At Expometeoritos, we handle outreach, talks, workshops, analyses, classification, and exhibitions of meteorites.
